Pith Number

pith:JRB2Q2IK

pith:2022:JRB2Q2IKNJMI5JZOB6CYCO3STV

not attested not anchored not stored refs pending

A Spectroscopic Road Map for Cosmic Frontier: DESI, DESI-II, Stage-5

Adam D. Myers, Adam S. Bolton, Alex Drlica-Wagner, Alex G. Kim, Alexie Leauthaud, Ana Bonaca, Anand Raichoor, Anthony Kremin, Antonella Palmese, Arjun Dey, Charles Baltay, Christophe Magneville, Christopher J. Miller, Christophe Yeche, Claire Poppett, Daniel Green, David Brooks, David J. Schlegel, Dionysios Karagiannis, Dragan Huterer, Dustin Lang, Elizabeth Buckley-Geer, Emmanuel Schaan, Eric V. Linder, Gaston Gutierrez, Greg Aldering, Greg Tarle, Guillermo A. Blanc, Hee-Jong Seo, Jason X. Prochaska, Jean-Paul Kneib, Jeffrey A. Newman, Joseph DeRose, Joseph Silber, Joshua D. Simon, Julien Guy, Juna A. Kollmeier, Leopoldo Infante, Marcelle Soares-Santos, Martin Landriau, Martin White, Michael E. Levi, Michael Schubnell, Monica Valluri, Nathalie Palanque-Delabrouille, Nikhil Padmanabhan, Noah J. Weaverdyck, Noah Sailer, Ofer Lahav, Patrick Jelinsky, Patrick McDonald, Paul Martini, Peter Doel, Peter E. Nugent, Risa H. Wechsler, Robert Besuner, Rongpu Zhou, Segev Benzvi, Simone Ferraro, Solange Ramirez, Stephen M. Kent, Uros Seljak, Xiaohui Fan, Zachary Slepian, Zheng Cai

arxiv:2209.03585 v1 · 2022-09-08 · astro-ph.CO · hep-ex

Open paper page JSON Open Graph Bundle Merged state Verified badge What is a Pith Number?

Add to your LaTeX paper

\usepackage{pith}
\pithnumber{JRB2Q2IKNJMI5JZOB6CYCO3STV}

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Record completeness

1 Bitcoin timestamp

2 Internet Archive

3 Author claim open · sign in to claim

4 Citations open

5 Replications open

✓ Portable graph bundle live · download bundle · merged state

The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Cited by

16 papers in Pith

Beyond {\Lambda}CDM with the SKA Observatory -- II: Unveiling the Secrets of the Early Universe

The 3D clustering of Lyman Alpha Emitters measured with DESI

Clustering of high-redshift quasars with DESI DR2

Optimization of Tessellation-based Statistics: Void Statistics

Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines

Receipt and verification

First computed	2026-07-05T04:55:43.574745Z
Builder	pith-number-builder-2026-05-17-v1
Signature	Pith Ed25519 (`pith-v1-2026-05`) · public key
Schema	pith-number/v1.0

Canonical hash

4c43a8690a6a588ea72e0f85813b729d567be7c13e0886b0d418b0d5dc3a0b96

Aliases

arxiv: 2209.03585 · arxiv_version: 2209.03585v1 · doi: 10.48550/arxiv.2209.03585 · pith_short_12: JRB2Q2IKNJMI · pith_short_16: JRB2Q2IKNJMI5JZO · pith_short_8: JRB2Q2IK

Agent API

Resolver JSON Graph JSON Events JSON Schema Signing key

Verify this Pith Number yourself

curl -sH 'Accept: application/ld+json' https://pith.science/pith/JRB2Q2IKNJMI5JZOB6CYCO3STV \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 4c43a8690a6a588ea72e0f85813b729d567be7c13e0886b0d418b0d5dc3a0b96

Canonical record JSON

{
  "metadata": {
    "abstract_canon_sha256": "e232f8b1cfee4a0045e98345c90d19497931de69081a69dbaef5a65d43ccd83a",
    "cross_cats_sorted": [
      "hep-ex"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.CO",
    "submitted_at": "2022-09-08T06:18:05Z",
    "title_canon_sha256": "64ada76ec4d75ba58854f5538e5ba7b66c000088d3e5c1ffb25a6136086a9e5a"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2209.03585",
    "kind": "arxiv",
    "version": 1
  }
}